Identifying mergers using non-parametric morphological classification at high redshifts
Robert Thompson, Romeel Dav\'e, Shuiyao Huang, Neal Katz

TL;DR
This study evaluates the effectiveness of non-parametric morphological indicators, especially asymmetry, in identifying major galaxy mergers at high redshifts ($z=2$ to 4) using cosmological simulations.
Contribution
It demonstrates that asymmetry is the most reliable morphological indicator for detecting major mergers at high redshifts, with specific thresholds improving detection accuracy.
Findings
High asymmetry values correlate strongly with recent major mergers.
Canonical asymmetry cut (A≥0.35) detects only about 10% of mergers.
Higher asymmetry thresholds (A≥0.8 or 1.5) improve merger identification.
Abstract
We investigate the time evolution of non-parametric morphological quantities and their relationship to major mergers between in high-resolution cosmological zoom simulations of disk galaxies that implement kinetic wind feedback, -based star formation, and minimal ISM pressurisation. We show that the resulting galaxies broadly match basic observed physical properties of objects. We measure the galaxies' concentrations (), asymmetries (), and () and coefficients, and correlate these with major merger events identified from the mass growth history. We find that high values of asymmetry provide the best indicator for identifying major mergers of mass ratio within our sample, with - merger classification only as effective for face-on systems and much less effective for edge-on or randomly-oriented galaxies. The…
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Taxonomy
TopicsAstronomy and Astrophysical Research · Stellar, planetary, and galactic studies · Galaxies: Formation, Evolution, Phenomena
